Earlier studies have shown that relaxation
effects are important to understand dissipative gravitational collapse
[1]}, [2]}, [3]}, [4]}, [5]}.
To study the temperature profiles,
we consider the transport equation for the metric
(REF ) given by [6]}, [1]}, [8]}
\(\tau h_{\mu }^{\nu }\dot{q}_{\nu }+q_{\mu }&=&-k\left( h_{\mu }^{\nu } \nabla _{\nu } T+T\dot{u}_{\mu } \right)\\\tau \left(qbs\right)_{,t}+q\,a\,b\,s&=&-\frac{k\left(aT \right)_{,r}}{bs}, \) 
